Surface characteristics of the Zhurong Mars rover traverse at Utopia Planitia

L Ding, R Zhou, T Yu, H Gao, H Yang, J Li, Y Yuan… - Nature …, 2022 - nature.com
Abstract China's Mars rover, Zhurong, touched down on Utopia Planitia in the northern
lowlands of Mars (109.925° E, 25.066° N) in May 2021, and has been conducting in situ …

Thermal and albedo map** of Mars during the Viking primary mission

HH Kieffer, TZ Martin, AR Peterfreund… - Journal of …, 1977 - Wiley Online Library
Measurements of Martian emission and reflection reveal wide variations of surface
properties and indicate the presence of a larger atmospheric contribution to the observed …

Buried palaeo-polygonal terrain detected underneath Utopia Planitia on Mars by the Zhurong radar

L Zhang, C Li, J Zhang, B Zhou, YYS Zhao, Y Liu… - Nature …, 2024 - nature.com
As the largest basin on Mars, Utopia Planitia has both experienced and recorded variations
of the Martian palaeoclimate. Layered subsurface structures have been identified by ground …

Possible ancient oceans on Mars: evidence from Mars Orbiter Laser Altimeter data

JW Head III, H Hiesinger, MA Ivanov, MA Kreslavsky… - Science, 1999 - science.org
High-resolution altimetric data define the detailed topography of the northern lowlands of
Mars, and a range of data is consistent with the hypothesis that a lowland-encircling …

Meteorological results from the surface of Mars: Viking 1 and 2

SL Hess, RM Henry, CB Leovy… - Journal of …, 1977 - Wiley Online Library
We deal here primarily with the surface meteorological data for both Viking landers during
the nominal missions (44 sols for lander 1 and 61 sols for lander 2). The diurnal patterns of …

Antarctic dry valleys: Microclimate zonation, variable geomorphic processes, and implications for assessing climate change on Mars

DR Marchant, JW Head III - Icarus, 2007 - Elsevier
The Antarctic Dry Valleys (ADV) are generally classified as a hyper-arid, cold-polar desert.
The region has long been considered an important terrestrial analog for Mars because of its …

Martian impact craters and emplacement of ejecta by surface flow

MH Carr, LS Crumpler, JA Cutts… - Journal of …, 1977 - Wiley Online Library
Several types of Martian impact craters have been recognized. The most common type, the
rampart crater, is distinctively different from lunar and Mercurian craters. It is typically …

Structure of the atmosphere of Mars in summer at mid‐latitudes

A Seiff, DB Kirk - Journal of Geophysical Research, 1977 - Wiley Online Library
The structure of Mars' atmosphere was measured in situ by instruments on board the two
Viking landers from an altitude of 120 km to near the surface. The two entries were …

Threshold windspeeds for sand on Mars: Wind tunnel simulations

R Greeley, R Leach, B White, J Iversen… - Geophysical …, 1980 - Wiley Online Library
Wind friction threshold speeds (u* t) for particle movement (saltation) were determined in a
wind tunnel operating at martian surface pressure with a 95 percent CO2 and 5 percent air …

Survival of endospores of Bacillus subtilis on spacecraft surfaces under simulated martian environments:: implications for the forward contamination of Mars

AC Schuerger, RL Mancinelli, RG Kern, LJ Rothschild… - Icarus, 2003 - Elsevier
Experiments were conducted in a Mars simulation chamber (MSC) to characterize the
survival of endospores of Bacillus subtilis under high UV irradiation and simulated martian …